Search Results - "Pan, Y. C."
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Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source
Published in Science (American Association for the Advancement of Science) (22-12-2017)“…On 17 August 2017, the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the Virgo interferometer detected gravitational waves (GWs) emanating…”
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Electromagnetic evidence that SSS17a is the result of a binary neutron star merger
Published in Science (American Association for the Advancement of Science) (22-12-2017)“…Eleven hours after the detection of gravitational wave source GW170817 by the Laser Interferometer Gravitational-Wave Observatory and Virgo Interferometers, an…”
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SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances
Published in The Astrophysical journal (01-12-2021)“…Abstract A spectral-energy distribution (SED) model for Type Ia supernovae (SNe Ia) is a critical tool for measuring precise and accurate distances across a…”
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Hypoxic lung cancer-secreted exosomal miR-23a increased angiogenesis and vascular permeability by targeting prolyl hydroxylase and tight junction protein ZO-1
Published in Oncogene (24-08-2017)“…Hypoxia plays a critical role during the evolution of malignant cells and tumour microenvironment (TME).Tumour-derived exosomes contain informative microRNAs…”
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Should Type Ia Supernova Distances Be Corrected for Their Local Environments?
Published in The Astrophysical journal (10-11-2018)“…Recent analyses suggest that distance residuals measured from Type Ia supernovae (SNe Ia) are correlated with local host galaxy properties within a few…”
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The Foundation Supernova Survey: Measuring Cosmological Parameters with Supernovae from a Single Telescope
Published in The Astrophysical journal (10-08-2019)“…Measurements of the dark energy equation-of-state parameter, w, have been limited by uncertainty in the selection effects and photometric calibration of z <…”
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Early spectra of the gravitational wave source GW170817: Evolution of a neutron star merger
Published in Science (American Association for the Advancement of Science) (22-12-2017)“…On 17 August 2017, Swope Supernova Survey 2017a (SSS17a) was discovered as the optical counterpart of the binary neutron star gravitational wave event…”
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Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters
Published in The Astrophysical journal (10-04-2018)“…We use 1169 Pan-STARRS supernovae (SNe) and 195 low-z (z < 0.1) SNe Ia to measure cosmological parameters. Though most Pan-STARRS SNe lack spectroscopic…”
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The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample
Published in The Astrophysical journal (01-06-2018)“…We present optical light curves, redshifts, and classifications for spectroscopically confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1)…”
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The host galaxies of Type Ia supernovae discovered by the Palomar Transient Factory
Published in Monthly notices of the Royal Astronomical Society (21-02-2014)“…We present spectroscopic observations of the host galaxies of 82 low-redshift Type Ia supernovae (SNe Ia) discovered by the Palomar Transient Factory. We…”
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500 days of SN 2013dy: spectra and photometry from the ultraviolet to the infrared
Published in Monthly notices of the Royal Astronomical Society (01-10-2015)“…SN 2013dy is a Type Ia supernova (SN Ia) for which we have compiled an extraordinary data set spanning from 0.1 to ∼ 500 d after explosion. We present 10…”
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Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis
Published in Science (American Association for the Advancement of Science) (22-12-2017)“…On 17 August 2017, gravitational waves (GWs) were detected from a binary neutron star merger, GW170817, along with a coincident short gamma-ray burst, GRB…”
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TYPE II SUPERNOVA ENERGETICS AND COMPARISON OF LIGHT CURVES TO SHOCK-COOLING MODELS
Published in The Astrophysical journal (20-03-2016)“…ABSTRACT During the first few days after explosion, Type II supernovae (SNe) are dominated by relatively simple physics. Theoretical predictions regarding…”
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Hydrogen-poor Superluminous Supernovae from the Pan-STARRS1 Medium Deep Survey
Published in The Astrophysical journal (10-01-2018)“…We present light curves and classification spectra of 17 hydrogen-poor superluminous supernovae (SLSNe) from the Pan-STARRS1 Medium Deep Survey (PS1 MDS). Our…”
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Nebular spectra and abundance tomography of the Type Ia supernova SN 2011fe: a normal SN Ia with a stable Fe core
Published in Monthly notices of the Royal Astronomical Society (01-07-2015)“…A series of optical and one near-infrared nebular spectra covering the first year of the Type Ia supernova SN 2011fe are presented and modelled. The density…”
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Exploring the spectral diversity of low-redshift Type Ia supernovae using the Palomar Transient Factory
Published in Monthly notices of the Royal Astronomical Society (11-11-2014)“…We present an investigation of the optical spectra of 264 low-redshift (z < 0.2) Type Ia supernovae (SNe Ia) discovered by the Palomar Transient Factory, an…”
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INTERACTING SUPERNOVAE AND SUPERNOVA IMPOSTORS: SN 2009ip, IS THIS THE END?
Published in The Astrophysical journal (10-04-2013)“…We report the results of a three-year-long dedicated monitoring campaign of a restless luminous blue variable (LBV) in NGC 7259. The object, named SN 2009ip,…”
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Cosmological Results from the RAISIN Survey: Using Type Ia Supernovae in the Near Infrared as a Novel Path to Measure the Dark Energy Equation of State
Published in The Astrophysical journal (01-07-2022)“…Abstract Type Ia supernovae (SNe Ia) are more precise standardizable candles when measured in the near-infrared (NIR) than in the optical. With this…”
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The unexpected, long-lasting, UV rebrightening of the superluminous supernova ASASSN-15lh
Published in Monthly notices of the Royal Astronomical Society (01-04-2017)“…Given its peak luminosity and early-time spectra, ASASSN-15lh was classified as the most luminous supernova ever discovered. Here, we report a UV rebrightening…”
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YSE-PZ: A Transient Survey Management Platform that Empowers the Human-in-the-loop
Published in Publications of the Astronomical Society of the Pacific (01-06-2023)“…Abstract The modern study of astrophysical transients has been transformed by an exponentially growing volume of data. Within the last decade, the transient…”
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